土星的低频辐射源
1Laboratoire d'Etudes Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris, Université Paris Sciences et Lettres, Centre National de la Recherche Scientifique, Sorbonne Université, Université Paris Diderot, Sorbonne Paris Cité, 5 Place Jules Janssen, 92195 Meudon, France. laurent.lamy@obspm.fr.
概括
土星
科学领域:
- 星球科学
- 太空物理
- 血物理
背景情况:
- 土星的千米辐射 (SKR) 是磁层过程的一个关键指标.
- 在现场测量对于了解极光射电源至关重要.
- 卡西尼的高倾斜轨道提供了独特的SKR源区域.
研究的目的:
- 研究土星千米辐射的现场生成机制.
- 将无线电发射与磁层中的等离子体和波状况相关联.
- 了解电子束和磁层密度在SKR生产中的作用.
主要方法:
- 使用卡西尼航天器的波浪和等离子体测量.
- 分析三次穿越高海拔地区的数据.
- 检查北方黎明侧磁层中的窄带无线电源.
主要成果:
- 在与极光圆相连的上升电流区域遇到10-20kHz的SKR源.
- 确定异常模式波是由旋转子巨星的不稳定引起的.
- 确定了6到12千电子伏特电子束作为排放源.
- 与极光磁场线相对观察到的准垂直辐射.
- 发现SKR源受到时间变化的磁层电子密度的强烈影响.
结论:
- 它是由来自高能电子束的自旋电磁束不稳定产生.
- 超常模式和近垂直发射是这些源的特征.
- 磁层电子密度变化在控制低频SKR源方面发挥着重要作用.
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